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A precessing Be disc as a possible model for occultation events in GX 304−1
UploadApplication of a physical continuum model to recent X-ray observations of accreting pulsars
UploadNuSTAR and Swift detection of a ~600 s QPO in 4U 0115+63
UploadLooking into the Theory of Pulsar Accretion: The Case of XTE J1946+274
UploadThe First Suzaku Observation of 4U 1538-522
UploadNo anticorrelation between cyclotron line energy and X-ray flux in 4U 0115+634
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